- Abstract:
-
Recent HI observations reveal that the discs of spiral galaxies are surrounded by extended gaseous haloes. This extra-planar gas reaches large distances (several kpc) from the disc and shows peculiar kinematics (low rotation and inflow). We have modelled the extra-planar gas as a continuous flow of material from the disc of a spiral galaxy into its halo region. The output of our models are pseudo-data cubes that can be directly compared to the HI data. We have applied these models to two spir...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1111/j.1365-2966.2005.09816.x
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- Journal:
- Mon.Not.Roy.Astron.Soc.
- Volume:
- 366
- Issue:
- 2
- Pages:
- 449-466
- Publication date:
- 2005-11-10
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:a33b2b9d-6c3b-4540-b8c9-756e7cb4b423
- Source identifiers:
-
28751
- Local pid:
- pubs:28751
- Language:
- English
- Keywords:
- Copyright date:
- 2005
- Notes:
-
19 pages, 20 figures, accepted for publication in MNRAS. High
resolution version available at
http://www-thphys.physics.ox.ac.uk/users/FilippoFraternali/interests.html
Journal article
A Dynamical Model for the Extra-planar Gas in Spiral Galaxies
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